From golub@head.cfa.harvard.edu Thu May 31 12:12:36 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.1.8 (2007-02-13) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.1.8 Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by auriga.ta3.sk (8.13.6/8.13.1) with ESMTP id l4VCBhL0019715 for ; Thu, 31 May 2007 12:12:34 GMT Received: from corona.cfa.harvard.edu (corona [131.142.41.245]) by head.cfa.harvard.edu (w/d) with ESMTP id l4VCBgid008806 for ; Thu, 31 May 2007 08:11:43 -0400 (EDT) From: Leon Golub Received: (from golub@localhost) by corona.cfa.harvard.edu (8.13.6/8.13.6) id l4VCBgF2010147 for choc@ta3.sk; Thu, 31 May 2007 08:11:42 -0400 (EDT) Date: Thu, 31 May 2007 08:11:42 -0400 (EDT) Message-Id: <200705311211.l4VCBgF2010147@corona.cfa.harvard.edu> To: choc@ta3.sk Subject: Re: Rybak - Hinode proposal X-Virus-Scanned: ClamAV version 0.90.2, clamav-milter version 0.90.2 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean Status: ROr Dear Dr. Rybak, I will print out your pdf file and look it over. If I have any comments or see any problems, I'll let you know. I will also sen this to the other relevant team members. Sincerely, Leon Golub From llundquist@cfa.harvard.edu Tue Jul 31 03:43:58 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00,HTML_MESSAGE autolearn=ham version=3.2.1 Received: from sprg-asmtp.ssl.berkeley.edu (sprg-asmtp.SSL.Berkeley.EDU [128.32.147.163]) by auriga.ta3.sk (8.13.6/8.13.6) with SMTP id l6V3h5Ka028238 for ; Tue, 31 Jul 2007 03:43:56 GMT Received: (qmail 2721 invoked from network); 30 Jul 2007 20:42:59 -0700 Received: from unknown (HELO ?133.74.8.102?) (loraine@133.74.8.102) by sprg-asmtp.ssl.berkeley.edu with SMTP; 30 Jul 2007 20:42:59 -0700 In-Reply-To: <8ec266b80707302038r34b4f6dfs5dadca5dc3c6884c@mail.gmail.com> References: <8ec266b80707302038r34b4f6dfs5dadca5dc3c6884c@mail.gmail.com> Mime-Version: 1.0 (Apple Message framework v752.3) Content-Type: multipart/alternative; boundary=Apple-Mail-25--759783914 Message-Id: Cc: sot_co@solar.isas.jaxa.jp, eis_co@solar.isas.jaxa.jp, "Dick Shine" , "Dawn Myers" , "Jan Rybak" From: Loraine Lundquist Subject: Re: HOP 24 quiet Sun prominence target & plan sot_co:xrt_co:eis_co: Date: Tue, 31 Jul 2007 12:42:09 +0900 To: xrt_co@solar.isas.jaxa.jp X-Mailer: Apple Mail (2.752.3) X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean Status: RO --Apple-Mail-25--759783914 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Dear Gary, I'm afraid XRT requires a week-long CCD bakeout and will not be able to participate. regards, Loraine ------------------------------------------------------------ Loraine Lundquist, Ph.D. Harvard Smithsonian Center for Astrophysics 60 Garden St., MS-58, Cambridge, MA 02138 (+1) 617-496-7964 (US) (+81) 090-6569-9964 (Japan) llundquist@cfa.harvard.edu ------------------------------------------------------------ On Jul 31, 2007, at 12:38 PM, Gary Kilper wrote: > Hello Hinode COs, > > There is a quiescent filament to the southwest of AR 10965 at about > [300", -500"] (on 7/31, 02:00) that has formed slowly and looks to > have stabilized in some sections, with some variability and possible > small eruptions in other sections. > > Assuming that it does not completely disappear, it will be targeted > via JOP 188 by SOHO & TRACE from 8/3 17:00 until 8/5 07:00 (excluding > 07:00-13:30 UT on 8/4, when JOP 189 will be running). > > For HOP 24 with Hinode, I would like to get observations when this > filament is still on the disk, and then when it is over the limb. > Those times would be: > > Disk: > 8/2, 17:00-24:00 > > Limb: > 8/4, 13:30-24:00 > 8/5, 00:00-07:00 > 8/5, 13:30-24:00 > > Previously I had talked with the COs in person about what I wanted > from their instruments, but here it is in writing (the HOP description > will be updated with this later): > > SOT: > disk: FG slot 12, H lc, CaH, G-b 2Kx2K 2x2, 30s (which is ROI2) > disk (if buffer is too full): FG slot 3, H lc 30sec, CaH and Gb > 120sec, 2Kx2K 2x2, ROI2 > limb: FG slot 14, H-a 2 wave for DG, CaH2Kx2K 2x2, 30s > > EIS: > Nothing too specific: Use a standard observing plan for quiet Sun > filament observations for the disk or limb. The wavelength list > should include Fe XII (195.12 A), Fe XIII (202.04 A), He II (256.32 > A), Fe XIV (264.78 A), and Fe XV (284.16 A). Depending on the > situation (i.e. raster size and data rate), more wavelengths would be > useful to fill out the temperature range -- especially on the lower > end. > > XRT: > Aluminum poly, 512"x512" field-of-view, 30 sec cadence. > > > I'm sending this a day early so I can field any questions there might > be. Also, note that JOP 188 will be finishing on August 5th, but the > observing window for HOP 24 is open-ended and should be listed as a > Target of Opportunity for quiet Sun prominences. > > > Thanks everyone! > Gary --Apple-Mail-25--759783914 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1 Dear Gary,=A0

I'm afraid XRT requires a = week-long CCD bakeout and will not be able to = participate.=A0

regards,=A0
Loraine=

Loraine Lundquist, Ph.D.
Harvard Smithsonian Center for = Astrophysics
60 Garden St., MS-58, Cambridge, = MA 02138
(+1) 617-496-7964 (US)
(+81) 090-6569-9964 (Japan)
llundquist@cfa.harvard.edu<= /DIV>
On Jul 31, = 2007, at 12:38 PM, Gary Kilper wrote:

Hello Hinode COs,

There is a = quiescent filament to the southwest of AR 10965 at about
[300", -500"] (on 7/31, 02:00) that has formed = slowly and looks to
have stabilized in some = sections, with some variability and possible
small eruptions in other sections.

Assuming = that it does not completely disappear, it will be targeted
via JOP 188 by SOHO & TRACE from 8/3 17:00 until = 8/5 07:00 (excluding
07:00-13:30 UT on 8/4, when = JOP 189 will be running).

For HOP 24 with Hinode, I would = like to get observations when this
filament is = still on the disk, and then when it is over the limb.
Those times would be:

8/2, 17:00-24:00

8/4, 13:30-24:00
8/5, 00:00-07:00
8/5, = 13:30-24:00

Previously I had talked with the COs in person about = what I wanted
from their instruments, but here = it is in writing (the HOP description
will be = updated with this later):

SOT:
disk: FG slot 12, H lc, CaH, G-b 2Kx2K 2x2, 30s = (which is ROI2)
disk (if buffer is too full): FG = slot 3, H lc 30sec, CaH and Gb
120sec, 2Kx2K = 2x2, ROI2
limb: FG slot 14, H-a 2 wave for = DG, CaH2Kx2K 2x2, 30s
EIS:
Nothing too specific: Use a standard observing plan = for quiet Sun
filament observations for the = disk or limb.=A0 The = wavelength list
should include Fe XII (195.12 = A), Fe XIII (202.04 A), He II (256.32
A), Fe = XIV (264.78 A), and Fe XV (284.16 A).=A0 Depending on the
situation (i.e. raster size and data rate), more = wavelengths would be
useful to fill out the = temperature range -- especially on the lower
end.

XRT:
Aluminum poly, 512"x512" field-of-view, 30 sec = cadence.


I'm = sending this a day early so I can field any questions there = might
be.=A0 Also, note that JOP 188 will = be finishing on August 5th, but the
observing = window for HOP 24 is open-ended and should be listed as a
Target of Opportunity for quiet Sun = prominences.


Thanks = everyone!
Gary
=





=

= --Apple-Mail-25--759783914-- From nishida@kwasan.kyoto-u.ac.jp Tue Aug 14 10:45:00 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from vesta.kusastro.kyoto-u.ac.jp (vesta.kusastro.kyoto-u.ac.jp [130.54.52.4]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7EAhmiC023959 for ; Tue, 14 Aug 2007 10:44:40 GMT Received: from [10.226.87.246] (h246.87.226.10.20865.vlan.kuins.net [10.226.87.246]) by vesta.kusastro.kyoto-u.ac.jp (Postfix) with ESMTP id DF2835280C3; Tue, 14 Aug 2007 19:43:46 +0900 (JST) Message-ID: <46C18762.1000705@kwasan.kyoto-u.ac.jp> Date: Tue, 14 Aug 2007 19:43:46 +0900 From: NISHIDA Keisuke User-Agent: Thunderbird 2.0.0.6 (Windows/20070728) MIME-Version: 1.0 To: Astrid Veronig Cc: xrt_co@solar.isas.jaxa.jp, dot_jop189_hop020@astro.sk Subject: Re: [xrt_co:01361] xrt_co: References: <200708130900.l7D90nT0021259@igam06ws.uni-graz.at> In-Reply-To: <200708130900.l7D90nT0021259@igam06ws.uni-graz.at> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 83 Status: RO Dear Veronig san, XRT is undergoing very long CCD bakeout due to instrumental reason. The length of the bakeout period has not yet been determined. Therefore, we may not be able to perform the requested operations with XRT at this time. Regards, Keisuke Nishida ---- Keisuke Nishida Kwasan Observatory, Graduate School of Science, Kyoto University Mail: nishida@kwasan.kyoto-u.ac.jp Fax: +81-75-593-9617 > Dear XRT planner, > > the period of our campaign HOP20 is approaching (18-23/8), > so I write to you to specify once more the details of > the XRT support for our DOT+Hinode_HOP20+SOHO_JOP189+TRACE > camapaign. The proposal had been sent in May to Dr. Golub. > > XRT study details: > - days 18-23/8 > - time 07:00-13:30 UT > - high cadence of the images using just one selected filter > - no binning > - loss-less compression > - no compensation of the solar rotation > - targets: - Active Region when located near the disk center (microflares) > - Quiet Sun near disk center when no activity is present there > (solar network) > - pointing: specified via e-mail a day in advance > - Selected mode depending on selected target/study: > a) Microflare mode (AR): 256x256 px, thin Be filter, exposure max. 1s with > AEC, cadence 10s > b) Network mode (QS): 384x384 px, thin-Al/Mesh, exposure max. 15s with > AEC, cadence 15s > > Information and details on our campaign can be found at > http://www.astro.sk/~choc/open/07_dot/07_dot.html > > Please let me know if the XRT studies will be performed as specified. > Furthermore, at what time (one day in advance?) do you need the target > information, in particular for the weekend 18,19,20/8 ? > > For coordinating reasons please send your reply also to > the following email address: > dot_jop189_hop020@astro.sk > > Thank you very much. I am looking forward to a good campaign! > > Best regards, > Astrid Veronig > > > ----------------------------------------------------------------------- > Astrid Veronig > Institute of Physics / IGAM > University of Graz Tel: ++43 (0)316 380 8609 > Universitaetsplatz 5 Fax: ++43 (0)316 380 9825 > A-8010 Graz, Austria E-mail: asv@igam.uni-graz.at > ----------------------------------------------------------------------- > > > From bish@cora.nwra.com Mon Aug 20 14:52:04 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from earth.cora.nwra.com (earth.cora.nwra.com [65.125.157.180]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7KEowhn027243 for ; Mon, 20 Aug 2007 14:51:50 GMT Received: from [10.123.10.61] (softbank126112016066.bbtec.net [126.112.16.66]) (authenticated bits=0) by earth.cora.nwra.com (8.13.8/8.13.8) with ESMTP id l7KEoqeC004684 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Mon, 20 Aug 2007 08:50:54 -0600 Message-ID: <46C9AA4B.3060509@cora.nwra.com> Date: Mon, 20 Aug 2007 08:50:51 -0600 From: Bish ishibashi Reply-To: bish@cora.nwra.com Organization: NWRA User-Agent: Thunderbird 1.5.0.12 (X11/20070530) MIME-Version: 1.0 To: xrt_co@solar.isas.jaxa.jp CC: jonathan cirtain , dot_jop189_hop020@astro.sk Subject: Re: [xrt_co:01484] Re: xrt_co: References: <1187619616.46c9a320edefc@igam01ws.kfunigraz.ac.at> <9D9256AA-B4A5-4648-9C65-13F312A5977A@cfa.harvard.edu> <1187620384.46c9a620ac53c@igam01ws.kfunigraz.ac.at> In-Reply-To: <1187620384.46c9a620ac53c@igam01ws.kfunigraz.ac.at> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 253 Status: RO Dear Astrid: If we terminate the bakeout before the conclusion of HOP20, XRT can be ready to perform micro-flare observation with thin-Be filter (Al-mesh observation may impose an instrumental problem at this point). EIS COs are keeping me informed on the target and timing at the daily meeting, so that helps. We'll let you know as soon as we resume normal operation and then begin HOP20 observations. Best regards, Bish Ishibashi (current XRT-CO) asv@IGAM06WS.uni-graz.at wrote: > Hello Jonathan, > > thanks for your prompt reply. I fully understand of course, there is no need for > apologies. I just didn't want to miss the opportunity of XRTs great observations > in case that they were possible, so I asked once more. > > Best regards, > Astrid > > >> Hello Astrid, >> We are still performing the CCD bakeout and this will continue for >> the next few days. I am afraid we will not complete this until after >> the 23 August. Please accept our apologies for missing the >> opportunity to collaborate with you at this time. >> Best regards, >> Jonathan Cirtain >> On Aug 20, 2007, at 10:20 AM, asv@igam06ws.uni-graz.at wrote: >> >>> Dear XRT CO, >>> >>> I just want to kindly ask whether XRT is still in CCD bakeout. Or, >>> if it is >>> maybe possible to support our HOP20 campaign. During the previous >>> discussion >>> (email below) the length of the bakeout was not yet determined. >>> >>> Thank you very much. >>> >>> Best regards, >>> Astrid Veronig >>> >>> >>>> Dear Veronig san, >>>> >>>> XRT is undergoing very long CCD bakeout due to instrumental reason. >>>> The length of the bakeout period has not yet been determined. >>>> Therefore, we may not be able to perform the requested operations >>>> with >>>> XRT at this time. >>>> >>>> Regards, >>>> Keisuke Nishida >>>> >>>> ---- >>>> Keisuke Nishida >>>> Kwasan Observatory, Graduate School of Science, Kyoto University >>>> Mail: nishida@kwasan.kyoto-u.ac.jp >>>> Fax: +81-75-593-9617 >>>> >>>> >>>>> Dear XRT planner, >>>>> >>>>> the period of our campaign HOP20 is approaching (18-23/8), >>>>> so I write to you to specify once more the details of >>>>> the XRT support for our DOT+Hinode_HOP20+SOHO_JOP189+TRACE >>>>> camapaign. The proposal had been sent in May to Dr. Golub. >>>>> >>>>> XRT study details: >>>>> - days 18-23/8 >>>>> - time 07:00-13:30 UT >>>>> - high cadence of the images using just one selected filter >>>>> - no binning >>>>> - loss-less compression >>>>> - no compensation of the solar rotation >>>>> - targets: - Active Region when located near the disk center >>>> (microflares) >>>>> - Quiet Sun near disk center when no activity is >>>>> present there >>>>> (solar network) >>>>> - pointing: specified via e-mail a day in advance >>>>> - Selected mode depending on selected target/study: >>>>> a) Microflare mode (AR): 256x256 px, thin Be filter, >>>>> exposure max. 1s >>>> with >>>>> AEC, cadence 10s >>>>> b) Network mode (QS): 384x384 px, thin-Al/Mesh, >>>>> exposure max. 15s >>>> with >>>>> AEC, cadence 15s >>>>> >>>>> Information and details on our campaign can be found at >>>>> http://www.astro.sk/~choc/open/07_dot/07_dot.html >>>>> >>>>> Please let me know if the XRT studies will be performed as >>>>> specified. >>>>> Furthermore, at what time (one day in advance?) do you need the >>>>> target >>>>> information, in particular for the weekend 18,19,20/8 ? >>>>> >>>>> For coordinating reasons please send your reply also to >>>>> the following email address: >>>>> dot_jop189_hop020@astro.sk >>>>> >>>>> Thank you very much. I am looking forward to a good campaign! >>>>> >>>>> Best regards, >>>>> Astrid Veronig >>>>> >>>>> >>>>> -------------------------------------------------------------------- >>>>> --- >>>>> Astrid Veronig >>>>> Institute of Physics / IGAM >>>>> University of Graz Tel: ++43 (0)316 380 8609 >>>>> Universitaetsplatz 5 Fax: ++43 (0)316 380 9825 >>>>> A-8010 Graz, Austria E-mail: asv@igam.uni-graz.at >>>>> -------------------------------------------------------------------- >>>>> --- >>>>> >>>>> >>>>> >>> >>> >>> >>> >>> (IGAM/UG) >>> ------------------------------------------------- >>> This mail sent through IMP: http://horde.org/imp/ >> > > > > (IGAM/UG) > ------------------------------------------------- > This mail sent through IMP: http://horde.org/imp/ -- "Bish" K. Ishibashi, Ph.D. NorthWest Research Associates, Inc. e bish@cora.nwra.com CoRA Division w 303-415-9701 x241 3380 Mitchell Lane f 303-415-9702 Boulder, CO 80303 U.S.A. h www.cora.nwra.com/~bish From bish@cora.nwra.com Wed Aug 22 14:47:55 2007 Return-Path: X-Spam-Checker-Version: SpamAssassin 3.2.1 (2007-05-02) on auriga.ta3.sk X-Spam-Level: X-Spam-Status: No, score=-2.6 required=5.0 tests=BAYES_00 autolearn=ham version=3.2.1 Received: from earth.cora.nwra.com (earth.cora.nwra.com [65.125.157.180]) by auriga.ta3.sk (8.13.6/8.13.6) with ESMTP id l7MEkqBb005437 for ; Wed, 22 Aug 2007 14:47:43 GMT Received: from [10.123.10.11] (softbank126112016066.bbtec.net [126.112.16.66]) (authenticated bits=0) by earth.cora.nwra.com (8.13.8/8.13.8) with ESMTP id l7MEkfcA031552 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NO); Wed, 22 Aug 2007 08:46:48 -0600 Message-ID: <46CC4C51.3010703@cora.nwra.com> Date: Wed, 22 Aug 2007 08:46:41 -0600 From: Bish ishibashi Reply-To: bish@cora.nwra.com Organization: NWRA User-Agent: Thunderbird 1.5.0.12 (X11/20070530) MIME-Version: 1.0 To: xrt_co@solar.isas.jaxa.jp CC: jonathan cirtain , dot_jop189_hop020@astro.sk Subject: Re: [xrt_co:01487] Re: xrt_co: References: <1187619616.46c9a320edefc@igam01ws.kfunigraz.ac.at> <9D9256AA-B4A5-4648-9C65-13F312A5977A@cfa.harvard.edu> <1187620384.46c9a620ac53c@igam01ws.kfunigraz.ac.at> <46C9AA4B.3060509@cora.nwra.com> <1187623813.46c9b38506a65@igam01ws.kfunigraz.ac.at> In-Reply-To: <1187623813.46c9b38506a65@igam01ws.kfunigraz.ac.at> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: ClamAV version 0.91.1, clamav-milter version 0.91.1 on localhost X-Virus-Scanned: by amavisd-milter (http://www.amavis.org/) X-Virus-Status: Clean X-Status: X-Keywords: X-UID: 314 Status: RO Dear Astrid: I regret to inform you that XRT was unable to perform any observation for HOP20 as we remain to bake the CCD. My sincere apologies, Bish asv@IGAM06WS.uni-graz.at wrote: > Dear Bish, > > thank you for your answer. And thanks also that you'll keep our HOP20 in mind, > in case that the XRT bakeout terminates bfore the end of our HOP. Thin Be-filter > would be fine. > > Best regards, > Astrid > >> Dear Astrid: >> >> If we terminate the bakeout before the conclusion of HOP20, >> XRT can be ready to perform micro-flare observation with >> thin-Be filter (Al-mesh observation may impose an instrumental >> problem at this point). >> >> EIS COs are keeping me informed on the target and timing >> at the daily meeting, so that helps. We'll let you know as >> soon as we resume normal operation and then begin HOP20 >> observations. >> >> Best regards, >> >> Bish Ishibashi (current XRT-CO) >> >> >> >> asv@IGAM06WS.uni-graz.at wrote: >>> Hello Jonathan, >>> >>> thanks for your prompt reply. I fully understand of course, there is no >> need for >>> apologies. I just didn't want to miss the opportunity of XRTs great >> observations >>> in case that they were possible, so I asked once more. >>> >>> Best regards, >>> Astrid >>> >>> >>>> Hello Astrid, >>>> We are still performing the CCD bakeout and this will continue for >>>> the next few days. I am afraid we will not complete this until after >>>> the 23 August. Please accept our apologies for missing the >>>> opportunity to collaborate with you at this time. >>>> Best regards, >>>> Jonathan Cirtain >>>> On Aug 20, 2007, at 10:20 AM, asv@igam06ws.uni-graz.at wrote: >>>> >>>>> Dear XRT CO, >>>>> >>>>> I just want to kindly ask whether XRT is still in CCD bakeout. Or, >>>>> if it is >>>>> maybe possible to support our HOP20 campaign. During the previous >>>>> discussion >>>>> (email below) the length of the bakeout was not yet determined. >>>>> >>>>> Thank you very much. >>>>> >>>>> Best regards, >>>>> Astrid Veronig >>>>> >>>>> >>>>>> Dear Veronig san, >>>>>> >>>>>> XRT is undergoing very long CCD bakeout due to instrumental reason. >>>>>> The length of the bakeout period has not yet been determined. >>>>>> Therefore, we may not be able to perform the requested operations >>>>>> with >>>>>> XRT at this time. >>>>>> >>>>>> Regards, >>>>>> Keisuke Nishida >>>>>> >>>>>> ---- >>>>>> Keisuke Nishida >>>>>> Kwasan Observatory, Graduate School of Science, Kyoto University >>>>>> Mail: nishida@kwasan.kyoto-u.ac.jp >>>>>> Fax: +81-75-593-9617 >>>>>> >>>>>> >>>>>>> Dear XRT planner, >>>>>>> >>>>>>> the period of our campaign HOP20 is approaching (18-23/8), >>>>>>> so I write to you to specify once more the details of >>>>>>> the XRT support for our DOT+Hinode_HOP20+SOHO_JOP189+TRACE >>>>>>> camapaign. The proposal had been sent in May to Dr. Golub. >>>>>>> >>>>>>> XRT study details: >>>>>>> - days 18-23/8 >>>>>>> - time 07:00-13:30 UT >>>>>>> - high cadence of the images using just one selected filter >>>>>>> - no binning >>>>>>> - loss-less compression >>>>>>> - no compensation of the solar rotation >>>>>>> - targets: - Active Region when located near the disk center >>>>>> (microflares) >>>>>>> - Quiet Sun near disk center when no activity is >>>>>>> present there >>>>>>> (solar network) >>>>>>> - pointing: specified via e-mail a day in advance >>>>>>> - Selected mode depending on selected target/study: >>>>>>> a) Microflare mode (AR): 256x256 px, thin Be filter, >>>>>>> exposure max. 1s >>>>>> with >>>>>>> AEC, cadence 10s >>>>>>> b) Network mode (QS): 384x384 px, thin-Al/Mesh, >>>>>>> exposure max. 15s >>>>>> with >>>>>>> AEC, cadence 15s >>>>>>> >>>>>>> Information and details on our campaign can be found at >>>>>>> http://www.astro.sk/~choc/open/07_dot/07_dot.html >>>>>>> >>>>>>> Please let me know if the XRT studies will be performed as >>>>>>> specified. >>>>>>> Furthermore, at what time (one day in advance?) do you need the >>>>>>> target >>>>>>> information, in particular for the weekend 18,19,20/8 ? >>>>>>> >>>>>>> For coordinating reasons please send your reply also to >>>>>>> the following email address: >>>>>>> dot_jop189_hop020@astro.sk >>>>>>> >>>>>>> Thank you very much. I am looking forward to a good campaign! >>>>>>> >>>>>>> Best regards, >>>>>>> Astrid Veronig >>>>>>> >>>>>>> >>>>>>> -------------------------------------------------------------------- >>>>>>> --- >>>>>>> Astrid Veronig >>>>>>> Institute of Physics / IGAM >>>>>>> University of Graz Tel: ++43 (0)316 380 8609 >>>>>>> Universitaetsplatz 5 Fax: ++43 (0)316 380 9825 >>>>>>> A-8010 Graz, Austria E-mail: asv@igam.uni-graz.at >>>>>>> -------------------------------------------------------------------- >>>>>>> --- >>>>>>> >>>>>>> >>>>>>> >>>>> >>>>> >>>>> >>>>> (IGAM/UG) >>>>> ------------------------------------------------- >>>>> This mail sent through IMP: http://horde.org/imp/ >>> >>> >>> (IGAM/UG) >>> ------------------------------------------------- >>> This mail sent through IMP: http://horde.org/imp/ >> -- >> "Bish" K. Ishibashi, Ph.D. >> >> NorthWest Research Associates, Inc. e bish@cora.nwra.com >> CoRA Division w 303-415-9701 x241 >> 3380 Mitchell Lane f 303-415-9702 >> Boulder, CO 80303 >> U.S.A. h www.cora.nwra.com/~bish >> > > > > (IGAM/UG) > ------------------------------------------------- > This mail sent through IMP: http://horde.org/imp/ -- "Bish" K. Ishibashi, Ph.D. NorthWest Research Associates, Inc. e bish@cora.nwra.com CoRA Division w 303-415-9701 x241 3380 Mitchell Lane f 303-415-9702 Boulder, CO 80303 U.S.A. h www.cora.nwra.com/~bish